论民事诉讼举证时限制度之确立

《关于民事诉讼证据的若干规定》确立了我国的民事证据举证时限制度,克服了证据随时提出主义所造成的证据突袭、恶意拖延诉讼、浪费司法资源、破坏生效判决既判力、损害诉讼程序安定性等缺陷,但现行法律规定在适用时仍有一些不足,妨碍了举证时限制度作用的发挥,对此予以归纳并提出相对应的完善措施。     

国内家用空调市场面临的挑战及对策分析

全面分析了国内家用空调市场所面临的困境与挑战;从市场细分的角度,有针对性的对国内家用空调业界在城镇市场、乡村市场、国际市场、高端市场应如何作为进行了思考,提出了具体的对策,提出了空调常态市场的概念。     

安徽省中小企业技术创新障碍与对策

中小企业对国家和地区的经济发展、社会稳定起着重要的作用.技术创新是企业发展的核心动力.中小企业要获得生存与发展,就必须持续地进行技术创新.安徽省中小企业的技术创新由于基础薄、起步晚,正面临创新主体错位、创新模式不当、信息化水平低、服务体系不完善等重重障碍.文章认为完善融资体系和技术创新服务体系、选择适当的技术创新模式以及加快培育中小企业集群式创新是推动安徽省中小企业技术创新、实现跨越式发展的有效路径.     

中小外贸企业经营机制创新分析

经营机制创新是中小型外贸企业摆脱困境的必由之路。针对目前面临的主要问题，从外部环境及企业自身经营机制缺陷方面对中小型外贸企业生存环境进行分析，并从实现经营机制创新角度探讨改善现状的方法，力图找出中小型外贸企业经营机制创新的突破点。     

rom 15 sel

with primary goat embryonic fibroblast showed no difference from traditional feederlayer-based culture method used in mouse and human. The putative primary EG colonies were multilayer clumps ofcompact cel     

对高频电路原理图绘制问题的探讨

本文结合Protel 99 SE在高频PCB设计中的应用,着重探讨在电路原理图的绘制上需要重点注意的一些特殊问题,并提出解决问题的方法,尽可能地减小对高频PCB设计的影响,提高PCB设计的效率。     

ASP技术在军事信息网络中的运用

通过介绍ASP技术,提出了利用其开发可靠、安全的军事信息网络Web站点的一般方法,并给出了ASP对数据库操作所使用的SQL语法,同时,介绍了SSL加密的方法.     

计算机帧时间对半实物仿真的影响

半实物仿真试验中,要求计算机帧时间与计算积分步长相一致,但在实际试验中不容易精确地做到。本文分析了这种不一致给半实物仿真试验带来的影响,给出了解决的办法,文章中还给出了一实例来说明。     

Field formation around negatively biased solar arrays in the LEO-plasma

Heavy emission caused by impacting plasma ions results in a fast discharging effect of the initially large surface potentials on the dielectric solar cells. This eventually counteracts the energization process of the plasma ions to the cover glasses and leaves no significant electric fields. Thus, with an existing thermal plasma, electrons are again able to reach dielectric surfaces. Strong localized electric fields of the order of several 10 kV/cm form near the interconnector-cover glass interface.     

EUV emission from normal galaxies

Using data from the Wide Field Camera EUV all-sky survey, we have established upper limits to the EUV flux from a sample of 30 bright, nearby, non-active spiral galaxies. These galaxies were chosen to be those most likely to be detected in the EUV on the basis of (i) low interstellar absorption within our own galaxy, (ii) brightness in other wavebands, (iii) high star formation activity, and (iv) proximity. The derived EUV upper limits are restrictive, and establish for the first time that the EUV flux escaping from galaxies does not constitute a major component of their bolometric luminosity, and in particular that it cannot be the sink for the energy injected into the interstellar medium by supernova explosions, as had been suggested following the failure to detect this power in the X-ray band.